A plane symmetric Bianchi type-I inflationary universe in general relativity

A plane symmetric homogeneous space-time in the presence of mass less scalar field with a flat potential is investigated. To get an inflationary universe, we have considered a flat region in which potential V is constant. Some physical and kinematical properties of the model are also discussed.

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Bibliographic Details
Published in:Astrophysics and space science 2009, Vol.319 (1), p.89-91
Main Authors: Reddy, D. R. K., Rao, S. Atchuta, Naidu, R. L.
Format: Article
Language:English
Subjects:
Astrobiology
Astronomy
Astrophysics
Astrophysics and Astroparticles
Cosmology
Kinematics
Observations and Techniques
Original Article
Physics
Physics and Astronomy
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
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Description
Summary:A plane symmetric homogeneous space-time in the presence of mass less scalar field with a flat potential is investigated. To get an inflationary universe, we have considered a flat region in which potential V is constant. Some physical and kinematical properties of the model are also discussed.
ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-008-9955-8